Fig. 7
Orbital solution of HD 95086 b assuming a coplanar configuration with the outer belt inclination (idisk = 130±3°, Ω = 98±3°, Su et al. 2017), an inner extent of the chaotic zone larger than 10 au, and an outer extent of the chaotic zone smaller than 106 au, that is, the inner boundary of the outer belt resolved by ALMA 1.3 mm observations.
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